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Results: 243
Number of items: 243
  • Open Access
    de Jong, J. A. (2000). On the origin of cyclical variability in the winds of massive stars. [Thesis, fully internal, Universiteit van Amsterdam].
  • Open Access
    Tauris, T. M., van den Heuvel, E. P. J., & Savonije, G. J. (2000). Formation of millisecond pulsars with heavy white dwarf companions; extreme mass transfer on subthermal timescales. Astrophysical Journal, 530, L93-L96. https://doi.org/10.1086/312496
  • Open Access
    van den Heuvel, E. P. J., Portegies Zwart, S. F., Bhattacharya, D., & Kaper, L. (2000). On the origin of the difference between the runaway velocities of the OB-supergiant X-ray binaries and the BE/X-ray binaries. Astronomy & Astrophysics, 364, 563-572. http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2000A%26A...364..563V&db_key=AST
  • Open Access
    Zaal, P. A. (2000). Observations and analysis of early-type stars at infrared wavelengths. [Thesis, fully internal, Universiteit van Amsterdam].
  • Tauris, T. M., Fender, R. P., van den Heuvel, E. P. J., Johnston, H. M., & Wu, K. (1999). Circinus X-1: Survivor of a high asymmetric supernova. Monthly Notices of the Royal Astronomical Society, 310, 1165-1169. https://doi.org/10.1046/j.1365-8711.1999.03068.x
  • van den Heuvel, E. R., & Klaassen, C. A. J. (1999). Bayes Convolution. International Statistical Review, 67, 287-299. https://doi.org/10.2307/1403707
  • Does, R. J. M. M., & van den Heuvel, E. R. (1999). Zakelijk Verbeter Programma. In P. de Mos, & D. van de Lagemaat (Eds.), Processen in beweging: Beheersen, vernieuwen, verantwoorden (pp. 47-60). Samsom.
  • van den Heuvel, E. P. J. (1999). Twee markante Nederlandse sterrenkundigen. Zenit, 26(1), 12-17.
  • Kahabka, P., van den Heuvel, E. P. J., & Rappaport, S. (1999). Supersoft x-ray stars and supernovae. Scientific American, 280-2, 28-35.
  • Li, X. D., Bombaci, I., Dey, M., & van den Heuvel, E. P. J. (1999). Is SAX J18084-3658 a strange star? Physical Review Letters, 83, 3776-3779. https://doi.org/10.1103/PhysRevLett.83.3776
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